Titlebook: Spiral Galaxies in the Near-IR; Proceedings of the E Dante Minniti,Hans-Walter Rix Conference proceedings 1996 Springer-Verlag Berlin Heide

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Photometric and Spectrophotometric Models in the NIRsed. One is a refined spectral synthesis of starbursts in the . band. Another model aims to predict synthetic spectra (continua and lines) and colors of starbursts and the Hubble Sequence from 220Å to 5μm.

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踉跄

装饰

Colour Gradients in the Optical and Near-IRroadband colours are easy to obtain for large samples of objects, making them ideal for statistical studies. In this paper I use the radial distribution of the colours in galaxies, which gives more insight into the local processes driving the global colour differences than integrated colours. Almost

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脱水

Alopecia-Areata

jagged

defile

Imaging of Local Group Bulge Populations in the Near Infrarede from a globular cluster-aged stellar population. Giants with .. < -5 are found in M31, M32, and M33, and the HST imaging strongly supports the idea that ground-based observers are not being confused by blended images of stars. On the other hand, a direct measurement of the age of the Galactic bulg

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Origin of Bulgesart of the spheroid formation process, that includes halo and bulge. In a more recently proposed scenario bulges form late, as a result of the dynamical evolution of a disk that is prone to develop a bar instability. Recent . and . results are reported that may help chosing among these two alternati